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Radial Velocities of CH Cyg Just as the Jets Appeared

  • Ewa Janaszak
  • Maciej Mikołajewski
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 145)

Abstract

The period of maximum brightness of CH Cygni which started in mid 1981 finished at the end of July 1984, when sudden drop by about 1 mag was observed (Fig.l). At the same time a radio outburst has occured and the jet structure has developed (Taylor et al.1986). The Toruń Observatory has recorded the spectra of CH Cygni just at this moment. Significant spectral variations, especially development of wide wings in Balmer emission lines have been found (Mikołajewski and Tomov 1985).

Keywords

Radial Velocity Absorption Line Sudden Drop Spectral Variation Maximum Brightness 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

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Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • Ewa Janaszak
    • 1
  • Maciej Mikołajewski
    • 2
  1. 1.Planetarium and Astronomical ObservatoryOlsztynPoland
  2. 2.Institute of AstronomyN.Copernicus UniversityToruńPoland

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